Pith Number
pith:YNYLUCTY
pith:2012:YNYLUCTYUXMW3E7DGNXZPMF2CX
not attested
not anchored
not stored
refs pending
Can filamentary accretion explain the orbital poles of the Milky Way satellites?
arxiv:1204.6039 v1 · 2012-04-26 · astro-ph.CO · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{YNYLUCTYUXMW3E7DGNXZPMF2CX}
Prints a linked badge after your title and injects PDF metadata. Compiles on arXiv. Learn more · Embed verified badge
Record completeness
1
Bitcoin timestamp
2
Internet Archive
3
Author claim
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claim
4
Citations
5
Replications
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Portable graph bundle live · download bundle · merged
state
The bundle contains the canonical record plus signed events. A mirror can host it anywhere and recompute the same
current state with the deterministic merge algorithm.
Receipt and verification
| First computed | 2026-05-18T01:57:43.627110Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
c370ba0a78a5d96d93e3336f97b0ba15d698a7f2987f4bcdf7e7dfa65493edde
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/YNYLUCTYUXMW3E7DGNXZPMF2CX \
| jq -c '.canonical_record' \
| python3 -c "import sys,json,hashlib; b=json.dumps(json.loads(sys.stdin.read()), sort_keys=True, separators=(',',':'), ensure_ascii=False).encode(); print(hashlib.sha256(b).hexdigest())"
# expect: c370ba0a78a5d96d93e3336f97b0ba15d698a7f2987f4bcdf7e7dfa65493edde
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "fbc93659d56a0e1f396034b0c8be019e37b9cff2a0b888f3fa39a91856b1ea13",
"cross_cats_sorted": [
"astro-ph.GA"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2012-04-26T20:00:00Z",
"title_canon_sha256": "d842aa3109662bae5a6cfd0e210320c29d95bb3cf683ac321cf2650992d38007"
},
"schema_version": "1.0",
"source": {
"id": "1204.6039",
"kind": "arxiv",
"version": 1
}
}